File:2MASS J0437 transit.jpg
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Summary
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Top: SpeX Prism spectrum of 2MASS J0437+2331 (blue) from Bowler et al. (2014), overplotted with PSO J060.3+25 (red) along with the field (black; Kirkpatrick et al. 2010) and vl-g (orange; Allers & Liu 2013a) standards of the same spectral type (L1) as PSO J060.3+25. All four spectra are normalized at the J-band peak. 2MASS J0437+2331 is notably redder than PSO J060.3+25 as well the L1 vl-g standard, while PSO J060.3+25 has colors similar to those of the field standard. Bottom: the same four spectra plotted separately for Y/J, H, and K bands, normalized separately for each band to compare the spectral shapes in each band. The two young Taurus objects and the L1 vl-g standard have similar shapes in all bands, distinct from the older field standard. From: https://iopscience.iop.org/article/10.3847/1538-4357/aa5df0
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 14:55, 18 October 2024 | | 1,350 × 1,550 (909 KB) | Foxy Husky (talk | contribs) | Top: SpeX Prism spectrum of 2MASS J0437+2331 (blue) from Bowler et al. (2014), overplotted with PSO J060.3+25 (red) along with the field (black; Kirkpatrick et al. 2010) and vl-g (orange; Allers & Liu 2013a) standards of the same spectral type (L1) as PSO J060.3+25. All four spectra are normalized at the J-band peak. 2MASS J0437+2331 is notably redder than PSO J060.3+25 as well the L1 vl-g standard, while PSO J060.3+25 has colors similar to those of the field standard. Bottom: the same four... |
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